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dc.contributor.CRUESPUNIVERSIDADE ESTADUAL DE CAMPINASpt_BR
dc.contributor.authorunicampEscobar, Carlos Ouriviopt_BR
dc.typeArtigopt_BR
dc.titleConstraints On Large Extra Dimensions From The Minos Experimenten
dc.titleConstraints on large extra dimensions from the MINOS experimentpt_BR
dc.contributor.authorAdamson, P.pt_BR
dc.contributor.authorAnghel, I.pt_BR
dc.contributor.authorAurisano, A.pt_BR
dc.contributor.authorBarr, G.pt_BR
dc.contributor.authorBishai, M.pt_BR
dc.contributor.authorBlake, A.pt_BR
dc.contributor.authorBock, G. J.pt_BR
dc.contributor.authorBogert, D.pt_BR
dc.contributor.authorCao, S. V.pt_BR
dc.contributor.authorCarroll, T. J.pt_BR
dc.contributor.authorCastromonte, C. M.pt_BR
dc.contributor.authorChen, R.pt_BR
dc.contributor.authorChildress, S.pt_BR
dc.contributor.authorCoelho, J. A. B.pt_BR
dc.contributor.authorCorwin, L.pt_BR
dc.contributor.authorCronin-Hennessy, D.pt_BR
dc.contributor.authorde Jong, J. K.pt_BR
dc.contributor.authorDe Rijck, S.pt_BR
dc.contributor.authorDevan, A. V.pt_BR
dc.contributor.authorDevenish, N. E.pt_BR
dc.contributor.authorDiwan, M. V.pt_BR
dc.contributor.authorEscobar, C. O.pt_BR
dc.contributor.authorEvans, J. J.pt_BR
dc.contributor.authorFalk, E.pt_BR
dc.contributor.authorFeldman, G. J.pt_BR
dc.contributor.authorFlanagan, W.pt_BR
dc.contributor.authorFrohne, M. V.pt_BR
dc.contributor.authorGabrielyan, M.pt_BR
dc.contributor.authorGallagher, H. R.pt_BR
dc.contributor.authorGermani, S.pt_BR
dc.contributor.authorGomes, R. A.pt_BR
dc.contributor.authorGoodman, M. C.pt_BR
dc.contributor.authorGouffon, P.pt_BR
dc.contributor.authorGraf, N.pt_BR
dc.contributor.authorGran, R.pt_BR
dc.contributor.authorGrzelak, K.pt_BR
dc.contributor.authorHabig, A.pt_BR
dc.contributor.authorHahn, S. R.pt_BR
dc.contributor.authorHartnell, J.pt_BR
dc.contributor.authorHatcher, R.pt_BR
dc.contributor.authorHolin, A.pt_BR
dc.contributor.authorHuang, J.pt_BR
dc.contributor.authorHylen, J.pt_BR
dc.contributor.authorIrwin, G. M.pt_BR
dc.contributor.authorIsvan, Z.pt_BR
dc.contributor.authorJames, C.pt_BR
dc.contributor.authorJensen, D.pt_BR
dc.contributor.authorKafka, T.pt_BR
dc.contributor.authorKasahara, S. M. S.pt_BR
dc.contributor.authorKoizumi, G.pt_BR
dc.contributor.authorKordosky, M.pt_BR
dc.contributor.authorKreymer, A.pt_BR
dc.contributor.authorLang, K.pt_BR
dc.contributor.authorLing, J.pt_BR
dc.contributor.authorLitchfield, P. J.pt_BR
dc.contributor.authorLucas, P.pt_BR
dc.contributor.authorMann, W. A.pt_BR
dc.contributor.authorMarshak, M. L.pt_BR
dc.contributor.authorMayer, N.pt_BR
dc.contributor.authorMcGivern, C.pt_BR
dc.contributor.authorMedeiros, M. M.pt_BR
dc.contributor.authorMehdiyev, R.pt_BR
dc.contributor.authorMeier, J. R.pt_BR
dc.contributor.authorMessier, M. D.pt_BR
dc.contributor.authorMiller, W. H.pt_BR
dc.contributor.authorMishra, S. R.pt_BR
dc.contributor.authorSher, S. M.pt_BR
dc.contributor.authorMoore, C. D.pt_BR
dc.contributor.authorMualem, L.pt_BR
dc.contributor.authorMusser, J.pt_BR
dc.contributor.authorNaples, D.pt_BR
dc.contributor.authorNelson, J. K.pt_BR
dc.contributor.authorNewman, H. B.pt_BR
dc.contributor.authorNichol, R. J.pt_BR
dc.contributor.authorNowak, J. A.pt_BR
dc.contributor.authorO'Connor, J.pt_BR
dc.contributor.authorOrchanian, M.pt_BR
dc.contributor.authorPahlka, R. B.pt_BR
dc.contributor.authorPaley, J.pt_BR
dc.contributor.authorPatterson, R. B.pt_BR
dc.contributor.authorPawloski, G.pt_BR
dc.contributor.authorPerch, A.pt_BR
dc.contributor.authorPfutzner, M. M.pt_BR
dc.contributor.authorPhan, D. D.pt_BR
dc.contributor.authorPhan-Budd, S.pt_BR
dc.contributor.authorPlunkett, R. K.pt_BR
dc.contributor.authorPoonthottathil, N.pt_BR
dc.contributor.authorQiu, X.pt_BR
dc.contributor.authorRadovic, A.pt_BR
dc.contributor.authorRebel, B.pt_BR
dc.contributor.authorRosenfeld, C.pt_BR
dc.contributor.authorRubin, H. A.pt_BR
dc.contributor.authorSail, P.pt_BR
dc.contributor.authorSanchez, M. C.pt_BR
dc.contributor.authorSchneps, J.pt_BR
dc.contributor.authorSchreckenberger, A.pt_BR
dc.contributor.authorSchreiner, P.pt_BR
dc.contributor.authorSharma, R.pt_BR
dc.contributor.authorSousa, A.pt_BR
dc.contributor.authorTagg, N.pt_BR
dc.contributor.authorTalaga, R. L.pt_BR
dc.contributor.authorThomas, J.pt_BR
dc.contributor.authorThomson, M. A.pt_BR
dc.contributor.authorTian, X.pt_BR
dc.contributor.authorTimmons, A.pt_BR
dc.contributor.authorTodd, J.pt_BR
dc.contributor.authorTognini, S. C.pt_BR
dc.contributor.authorToner, R.pt_BR
dc.contributor.authorTorretta, D.pt_BR
dc.contributor.authorTzanakos, G.pt_BR
dc.contributor.authorUrheim, J.pt_BR
dc.contributor.authorVahle, P.pt_BR
dc.contributor.authorViren, B.pt_BR
dc.contributor.authorWeber, A.pt_BR
dc.contributor.authorWebb, R. C.pt_BR
dc.contributor.authorWhite, C.pt_BR
dc.contributor.authorWhitehead, L.pt_BR
dc.contributor.authorWhitehead, L. H.pt_BR
dc.contributor.authorWojcicki, S. G.pt_BR
dc.contributor.authorZwaska, R.pt_BR
dc.subjectNeutrino Oscillationsen
dc.subjectLepton Chargeen
dc.subjectMatteren
dc.subjectMassen
dc.subjectOscilações de neutrinos, Detectores, Modelo padrão (Física nuclear)pt_BR
dc.subject.otherlanguageNeutrinos oscillations, Detectors, Standard model (Nuclear physics)pt_BR
dc.description.abstractWe report new constraints on the size of large extra dimensions from data collected by the MINOS experiment between 2005 and 2012. Our analysis employs a model in which sterile neutrinos arise as Kaluza-Klein states in large extra dimensions and thus modify the neutrino oscillation probabilities due to mixing between active and sterile neutrino states. Using Fermilab's Neutrinos at the Main Injector beam exposure of 10.56 x 10(20) protons on target, we combine muon neutrino charged current and neutral current data sets from the Near and Far Detectors and observe no evidence for deviations from standard three-flavor neutrino oscillations. The ratios of reconstructed energy spectra in the two detectors constrain the size of large extra dimensions to be smaller than 0.45 mu m at 90% C.L. in the limit of a vanishing lightest active neutrino mass. Stronger limits are obtained for nonvanishing masses.en
dc.description.abstractWe report new constraints on the size of large extra dimensions from data collected by the MINOS experiment between 2005 and 2012. Our analysis employs a model in which sterile neutrinos arise as Kaluza-Klein states in large extra dimensions and thus modify the neutrino oscillation probabilities due to mixing between active and sterile neutrino states. Using Fermilab's Neutrinos at the Main Injector beam exposure of 10.56 x 10(20) protons on target, we combine muon neutrino charged current and neutral current data sets from the Near and Far Detectors and observe no evidence for deviations from standard three-flavor neutrino oscillations. The ratios of reconstructed energy spectra in the two detectors constrain the size of large extra dimensions to be smaller than 0.45 mu m at 90% C.L. in the limit of a vanishing lightest active neutrino mass. Stronger limits are obtained for nonvanishing masses.pt_BR
dc.relation.ispartofPhysical review. D, Covering particles, fields, gravitation, and cosmologypt_BR
dc.relation.ispartofabbreviationPhys. rev. Dpt_BR
dc.publisher.cityCollege Park, MDpt_BR
dc.publisher.countryEstados Unidospt_BR
dc.publisherAmerican Physical Societypt_BR
dc.date.issued2016pt_BR
dc.date.monthofcirculationDec.pt_BR
dc.identifier.citationPhysical Review D. Amer Physical Soc, v. 94, p. , 2016.pt_BR
dc.language.isoengpt_BR
dc.description.volume94pt_BR
dc.description.issuenumber11pt_BR
dc.description.firstpage1pt_BR
dc.description.lastpage7pt_BR
dc.rightsabertopt_BR
dc.sourceWOSpt_BR
dc.identifier.issn2470-0010pt_BR
dc.identifier.eissn2470-0029pt_BR
dc.identifier.doi10.1103/PhysRevD.94.111101pt_BR
dc.identifier.urlhttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.94.111101pt_BR
dc.description.sponsorshipFAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOpt_BR
dc.description.sponsorshipCNPQ - CONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICOpt_BR
dc.description.sponsorshipCAPES - COORDENAÇÃO DE APERFEIÇOAMENTO DE PESSOAL DE NÍVEL SUPERIORpt_BR
dc.description.sponsorship1FAPESP - FUNDAÇÃO DE AMPARO À PESQUISA DO ESTADO DE SÃO PAULOpt_BR
dc.description.sponsorship1CNPQ - CONSELHO NACIONAL DE DESENVOLVIMENTO CIENTÍFICO E TECNOLÓGICOpt_BR
dc.description.sponsorship1CAPES - COORDENAÇÃO DE APERFEIÇOAMENTO DE PESSOAL DE NÍVEL SUPERIORpt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.description.sponsordocumentnumberSem informaçãopt_BR
dc.date.available2017-11-13T13:46:04Z-
dc.date.accessioned2017-11-13T13:46:04Z-
dc.description.provenanceMade available in DSpace on 2017-11-13T13:46:04Z (GMT). No. of bitstreams: 1 000390275600001.pdf: 377378 bytes, checksum: 8a21b4ef682d8e8eea83f888d2499c01 (MD5) Previous issue date: 2016 Bitstreams deleted on 2020-09-02T13:42:26Z: 000390275600001.pdf,. Added 1 bitstream(s) on 2020-09-02T13:46:48Z : No. of bitstreams: 1 000390275600001.pdf: 460122 bytes, checksum: 5bbd43b39e21a2f54955f615902ef429 (MD5)en
dc.identifier.urihttp://repositorio.unicamp.br/jspui/handle/REPOSIP/329123-
dc.contributor.departmentDepartamento de Raios Cósmicos e Cronologiapt_BR
dc.contributor.unidadeInstituto de Física Gleb Wataghinpt_BR
dc.identifier.source000390275600001pt_BR
dc.creator.orcidSem informaçãopt_BR
dc.type.formArtigopt_BR
dc.identifier.articleid111101pt_BR
dc.description.sponsorNoteThis work was supported by the U.S. Department of Energy, the United Kingdom Science and Technology Facilities Council, the U.S. National Science Foundation, the State and University of Minnesota, and Brazil’s Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP), Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), and Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES). We are grateful to the Minnesota Department of Natural Resources and the personnel of the Soudan Laboratory and Fermilab. We thank the Texas Advanced Computing Center at The University of Texas at Austin for the provision of computing resources. We wish to thank P. A. N. Machado for providing insightful comments on the LED model.pt_BR
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